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EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN)

CERN-PH-EP-2013-053 LHCb-PAPER-2013-011 27 May 2013

Precision measurement of D differences

The LHCb collaboration†

Abstract Using three- and four-body decays of D produced in semileptonic b- decays, precision measurements of mass differences are made together with a measurement of the D0 mass. The measurements are based on a dataset corresponding to an integrated luminosity of 1.0 fb−1 collected in pp collisions at 7 TeV. Using the decay D0 → K+K−K−π+, the D0 mass is measured to be M(D0) = 1864.75 ± 0.15 (stat) ± 0.11 (syst) MeV/c2. The mass differences M(D+) − M(D0) = 4.76 ± 0.12 (stat) ± 0.07 (syst) MeV/c2, + + 2 M(Ds ) − M(D ) = 98.68 ± 0.03 (stat) ± 0.04 (syst) MeV/c arXiv:1304.6865v3 [hep-ex] 24 Jun 2013 0 + − + − + + − + are measured using the D → K K π π and D(s) → K K π modes.

Submitted to JHEP c CERN on behalf of the LHCb collaboration, license CC-BY-3.0.

†Authors are listed on the following pages. ii LHCb collaboration

R. Aaij40, C. Abellan Beteta35,n, B. Adeva36, M. Adinolfi45, C. Adrover6, A. Affolder51, Z. Ajaltouni5, J. Albrecht9, F. Alessio37, M. Alexander50, S. Ali40, G. Alkhazov29, P. Alvarez Cartelle36, A.A. Alves Jr24,37, S. Amato2, S. Amerio21, Y. Amhis7, L. Anderlini17,f , J. Anderson39, R. Andreassen56, R.B. Appleby53, O. Aquines Gutierrez10, F. Archilli18, A. Artamonov 34, M. Artuso57, E. Aslanides6, G. Auriemma24,m, S. Bachmann11, J.J. Back47, C. Baesso58, V. Balagura30, W. Baldini16, R.J. Barlow53, C. Barschel37, S. Barsuk7, W. Barter46, Th. Bauer40, A. Bay38, J. Beddow50, F. Bedeschi22, I. Bediaga1, S. Belogurov30, K. Belous34, I. Belyaev30, E. Ben-Haim8, M. Benayoun8, G. Bencivenni18, S. Benson49, J. Benton45, A. Berezhnoy31, R. Bernet39, M.-O. Bettler46, M. van Beuzekom40, A. Bien11, S. Bifani44, T. Bird53, A. Bizzeti17,h, P.M. Bjørnstad53, T. Blake37, F. Blanc38, J. Blouw11, S. Blusk57, V. Bocci24, A. Bondar33, N. Bondar29, W. Bonivento15, S. Borghi53, A. Borgia57, T.J.V. Bowcock51, E. Bowen39, C. Bozzi16, T. Brambach9, J. van den Brand41, J. Bressieux38, D. Brett53, M. Britsch10, T. Britton57, N.H. Brook45, H. Brown51, I. Burducea28, A. Bursche39, G. Busetto21,q, J. Buytaert37, S. Cadeddu15, O. Callot7, M. Calvi20,j, M. Calvo Gomez35,n, A. Camboni35, P. Campana18,37, D. Campora Perez37, A. Carbone14,c, G. Carboni23,k, R. Cardinale19,i, A. Cardini15, H. Carranza-Mejia49, L. Carson52, K. Carvalho Akiba2, G. Casse51, M. Cattaneo37, Ch. Cauet9, M. Charles54, Ph. Charpentier37, P. Chen3,38, N. Chiapolini39, M. Chrzaszcz 25, K. Ciba37, X. Cid Vidal37, G. Ciezarek52, P.E.L. Clarke49, M. Clemencic37, H.V. Cliff46, J. Closier37, C. Coca28, V. Coco40, J. Cogan6, E. Cogneras5, P. Collins37, A. Comerma-Montells35, A. Contu15,37, A. Cook45, M. Coombes45, S. Coquereau8, G. Corti37, B. Couturier37, G.A. Cowan49, D.C. Craik47, S. Cunliffe52, R. Currie49, C. D’Ambrosio37, P. David8, P.N.Y. David40, A. Davis56, I. De Bonis4, K. De Bruyn40, S. De Capua53, M. De Cian39, J.M. De Miranda1, L. De Paula2, W. De Silva56, P. De Simone18, D. Decamp4, M. Deckenhoff9, L. Del Buono8, D. Derkach14, O. Deschamps5, F. Dettori41, A. Di Canto11, H. Dijkstra37, M. Dogaru28, S. Donleavy51, F. Dordei11, A. Dosil Su´arez36, D. Dossett47, A. Dovbnya42, F. Dupertuis38, R. Dzhelyadin34, A. Dziurda25, A. Dzyuba29, S. Easo48,37, U. Egede52, V. Egorychev30, S. Eidelman33, D. van Eijk40, S. Eisenhardt49, U. Eitschberger9, R. Ekelhof9, L. Eklund50,37, I. El Rifai5, Ch. Elsasser39, D. Elsby44, A. Falabella14,e, C. F¨arber11, G. Fardell49, C. Farinelli40, S. Farry12, V. Fave38, D. Ferguson49, V. Fernandez Albor36, F. Ferreira Rodrigues1, M. Ferro-Luzzi37, S. Filippov32, M. Fiore16, C. Fitzpatrick37, M. Fontana10, F. Fontanelli19,i, R. Forty37, O. Francisco2, M. Frank37, C. Frei37, M. Frosini17,f , S. Furcas20, E. Furfaro23,k, A. Gallas Torreira36, D. Galli14,c, M. Gandelman2, P. Gandini57, Y. Gao3, J. Garofoli57, P. Garosi53, J. Garra Tico46, L. Garrido35, C. Gaspar37, R. Gauld54, E. Gersabeck11, M. Gersabeck53, T. Gershon47,37, Ph. Ghez4, V. Gibson46, V.V. Gligorov37, C. G¨obel58, D. Golubkov30, A. Golutvin52,30,37, A. Gomes2, H. Gordon54, M. Grabalosa G´andara5, R. Graciani Diaz35, L.A. Granado Cardoso37, E. Graug´es35, G. Graziani17, A. Grecu28, E. Greening54, S. Gregson46, O. Gr¨unberg59, B. Gui57, E. Gushchin32, Yu. Guz34,37, T. Gys37, C. Hadjivasiliou57, G. Haefeli38, C. Haen37, S.C. Haines46, S. Hall52, T. Hampson45, S. Hansmann-Menzemer11, N. Harnew54, S.T. Harnew45, J. Harrison53, T. Hartmann59, J. He37, V. Heijne40, K. Hennessy51, P. Henrard5, J.A. Hernando Morata36, E. van Herwijnen37, E. Hicks51, D. Hill54, M. Hoballah5, C. Hombach53, P. Hopchev4, W. Hulsbergen40, P. Hunt54, T. Huse51, N. Hussain54, D. Hutchcroft51, D. Hynds50, V. Iakovenko43, M. Idzik26, P. Ilten12, R. Jacobsson37, A. Jaeger11, E. Jans40, P. Jaton38, F. Jing3, M. John54, D. Johnson54, C.R. Jones46, B. Jost37, M. Kaballo9,

iii S. Kandybei42, M. Karacson37, T.M. Karbach37, I.R. Kenyon44, U. Kerzel37, T. Ketel41, A. Keune38, B. Khanji20, O. Kochebina7, I. Komarov38, R.F. Koopman41, P. Koppenburg40, M. Korolev31, A. Kozlinskiy40, L. Kravchuk32, K. Kreplin11, M. Kreps47, G. Krocker11, P. Krokovny33, F. Kruse9, M. Kucharczyk20,25,j, V. Kudryavtsev33, T. Kvaratskheliya30,37, V.N. La Thi38, D. Lacarrere37, G. Lafferty53, A. Lai15, D. Lambert49, R.W. Lambert41, E. Lanciotti37, G. Lanfranchi18, C. Langenbruch37, T. Latham47, C. Lazzeroni44, R. Le Gac6, J. van Leerdam40, J.-P. Lees4, R. Lef`evre5, A. Leflat31, J. Lefran¸cois7, S. Leo22, O. Leroy6, T. Lesiak25, B. Leverington11, Y. Li3, L. Li Gioi5, M. Liles51, R. Lindner37, C. Linn11, B. Liu3, G. Liu37, S. Lohn37, I. Longstaff50, J.H. Lopes2, E. Lopez Asamar35, N. Lopez-March38, H. Lu3, D. Lucchesi21,q, J. Luisier38, H. Luo49, F. Machefert7, I.V. Machikhiliyan4,30, F. Maciuc28, O. Maev29,37, S. Malde54, G. Manca15,d, G. Mancinelli6, U. Marconi14, R. M¨arki38, J. Marks11, G. Martellotti24, A. Martens8, L. Martin54, A. Mart´ın S´anchez7, M. Martinelli40, D. Martinez Santos41, D. Martins Tostes2, A. Massafferri1, R. Matev37, Z. Mathe37, C. Matteuzzi20, E. Maurice6, A. Mazurov16,32,37,e, J. McCarthy44, A. McNab53, R. McNulty12, B. Meadows56,54, F. Meier9, M. Meissner11, M. Merk40, D.A. Milanes8, M.-N. Minard4, J. Molina Rodriguez58, S. Monteil5, D. Moran53, P. Morawski25, M.J. Morello22,s, R. Mountain57, I. Mous40, F. Muheim49, K. M¨uller39, R. Muresan28, B. Muryn26, B. Muster38, P. Naik45, T. Nakada38, R. Nandakumar48, I. Nasteva1, M. Needham49, N. Neufeld37, A.D. Nguyen38, T.D. Nguyen38, C. Nguyen-Mau38,p, M. Nicol7, V. Niess5, R. Niet9, N. Nikitin31, T. Nikodem11, A. Nomerotski54, A. Novoselov34, A. Oblakowska-Mucha26, V. Obraztsov34, S. Oggero40, S. Ogilvy50, O. Okhrimenko43, R. Oldeman15,d, M. Orlandea28, J.M. Otalora Goicochea2, P. Owen52, A. Oyanguren 35,o, B.K. Pal57, A. Palano13,b, M. Palutan18, J. Panman37, A. Papanestis48, M. Pappagallo50, C. Parkes53, C.J. Parkinson52, G. Passaleva17, G.D. Patel51, M. Patel52, G.N. Patrick48, C. Patrignani19,i, C. Pavel-Nicorescu28, A. Pazos Alvarez36, A. Pellegrino40, G. Penso24,l, M. Pepe Altarelli37, S. Perazzini14,c, D.L. Perego20,j, E. Perez Trigo36, A. P´erez-CaleroYzquierdo35, P. Perret5, M. Perrin-Terrin6, G. Pessina20, K. Petridis52, A. Petrolini19,i, A. Phan57, E. Picatoste Olloqui35, B. Pietrzyk4, T. Pilaˇr47, D. Pinci24, S. Playfer49, M. Plo Casasus36, F. Polci8, G. Polok25, A. Poluektov47,33, E. Polycarpo2, D. Popov10, B. Popovici28, C. Potterat35, A. Powell54, J. Prisciandaro38, V. Pugatch43, A. Puig Navarro38, G. Punzi22,r, W. Qian4, J.H. Rademacker45, B. Rakotomiaramanana38, M.S. Rangel2, I. Raniuk42, N. Rauschmayr37, G. Raven41, S. Redford54, M.M. Reid47, A.C. dos Reis1, S. Ricciardi48, A. Richards52, K. Rinnert51, V. Rives Molina35, D.A. Roa Romero5, P. Robbe7, E. Rodrigues53, P. Rodriguez Perez36, S. Roiser37, V. Romanovsky34, A. Romero Vidal36, J. Rouvinet38, T. Ruf37, F. Ruffini22, H. Ruiz35, P. Ruiz Valls35,o, G. Sabatino24,k, J.J. Saborido Silva36, N. Sagidova29, P. Sail50, B. Saitta15,d, C. Salzmann39, B. Sanmartin Sedes36, M. Sannino19,i, R. Santacesaria24, C. Santamarina Rios36, E. Santovetti23,k, M. Sapunov6, A. Sarti18,l, C. Satriano24,m, A. Satta23, M. Savrie16,e, D. Savrina30,31, P. Schaack52, M. Schiller41, H. Schindler37, M. Schlupp9, M. Schmelling10, B. Schmidt37, O. Schneider38, A. Schopper37, M.-H. Schune7, R. Schwemmer37, B. Sciascia18, A. Sciubba24, M. Seco36, A. Semennikov30, K. Senderowska26, I. Sepp52, N. Serra39, J. Serrano6, P. Seyfert11, M. Shapkin34, I. Shapoval16,42, P. Shatalov30, Y. Shcheglov29, T. Shears51,37, L. Shekhtman33, O. Shevchenko42, V. Shevchenko30, A. Shires52, R. Silva Coutinho47, T. Skwarnicki57, N.A. Smith51, E. Smith54,48, M. Smith53, M.D. Sokoloff56, F.J.P. Soler50, F. Soomro18, D. Souza45, B. Souza De Paula2, B. Spaan9, A. Sparkes49, P. Spradlin50, F. Stagni37, S. Stahl11, O. Steinkamp39, S. Stoica28, S. Stone57, B. Storaci39, M. Straticiuc28, U. Straumann39, V.K. Subbiah37, S. Swientek9, V. Syropoulos41,

iv M. Szczekowski27, P. Szczypka38,37, T. Szumlak26, S. T’Jampens4, M. Teklishyn7, E. Teodorescu28, F. Teubert37, C. Thomas54, E. Thomas37, J. van Tilburg11, V. Tisserand4, M. Tobin38, S. Tolk41, D. Tonelli37, S. Topp-Joergensen54, N. Torr54, E. Tournefier4,52, S. Tourneur38, M.T. Tran38, M. Tresch39, A. Tsaregorodtsev6, P. Tsopelas40, N. Tuning40, M. Ubeda Garcia37, A. Ukleja27, D. Urner53, U. Uwer11, V. Vagnoni14, G. Valenti14, R. Vazquez Gomez35, P. Vazquez Regueiro36, S. Vecchi16, J.J. Velthuis45, M. Veltri17,g, G. Veneziano38, M. Vesterinen37, B. Viaud7, D. Vieira2, X. Vilasis-Cardona35,n, A. Vollhardt39, D. Volyanskyy10, D. Voong45, A. Vorobyev29, V. Vorobyev33, C. Voß59, H. Voss10, R. Waldi59, R. Wallace12, S. Wandernoth11, J. Wang57, D.R. Ward46, N.K. Watson44, A.D. Webber53, D. Websdale52, M. Whitehead47, J. Wicht37, J. Wiechczynski25, D. Wiedner11, L. Wiggers40, G. Wilkinson54, M.P. Williams47,48, M. Williams55, F.F. Wilson48, J. Wishahi9, M. Witek25, S.A. Wotton46, S. Wright46, S. Wu3, K. Wyllie37, Y. Xie49,37, F. Xing54, Z. Xing57, Z. Yang3, R. Young49, X. Yuan3, O. Yushchenko34, M. Zangoli14, M. Zavertyaev10,a, F. Zhang3, L. Zhang57, W.C. Zhang12, Y. Zhang3, A. Zhelezov11, A. Zhokhov30, L. Zhong3, A. Zvyagin37.

1Centro Brasileiro de Pesquisas F´ısicas (CBPF), Rio de Janeiro, Brazil 2Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil 3Center for High Energy Physics, Tsinghua University, Beijing, China 4LAPP, Universit´ede Savoie, CNRS/IN2P3, Annecy-Le-Vieux, France 5Clermont Universit´e,Universit´eBlaise Pascal, CNRS/IN2P3, LPC, Clermont-Ferrand, France 6CPPM, Aix-Marseille Universit´e,CNRS/IN2P3, Marseille, France 7LAL, Universit´eParis-Sud, CNRS/IN2P3, Orsay, France 8LPNHE, Universit´ePierre et Marie Curie, Universit´eParis Diderot, CNRS/IN2P3, Paris, France 9Fakult¨atPhysik, Technische Universit¨atDortmund, Dortmund, Germany 10Max-Planck-Institut f¨urKernphysik (MPIK), Heidelberg, Germany 11Physikalisches Institut, Ruprecht-Karls-Universit¨atHeidelberg, Heidelberg, Germany 12School of Physics, University College Dublin, Dublin, Ireland 13Sezione INFN di Bari, Bari, 14Sezione INFN di Bologna, Bologna, Italy 15Sezione INFN di Cagliari, Cagliari, Italy 16Sezione INFN di Ferrara, Ferrara, Italy 17Sezione INFN di Firenze, Firenze, Italy 18Laboratori Nazionali dell’INFN di Frascati, Frascati, Italy 19Sezione INFN di Genova, Genova, Italy 20Sezione INFN di Milano Bicocca, Milano, Italy 21Sezione INFN di Padova, Padova, Italy 22Sezione INFN di Pisa, Pisa, Italy 23Sezione INFN di Roma Tor Vergata, Roma, Italy 24Sezione INFN di Roma La Sapienza, Roma, Italy 25Henryk Niewodniczanski Institute of Polish Academy of Sciences, Krak´ow,Poland 26AGH - University of Science and Technology, Faculty of Physics and Applied Computer Science, Krak´ow,Poland 27National Center for Nuclear Research (NCBJ), Warsaw, Poland 28Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania 29Petersburg Nuclear Physics Institute (PNPI), Gatchina, Russia 30Institute of Theoretical and Experimental Physics (ITEP), Moscow, Russia 31Institute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, Russia 32Institute for Nuclear Research of the Russian Academy of Sciences (INR RAN), Moscow, Russia 33Budker Institute of Nuclear Physics (SB RAS) and Novosibirsk State University, Novosibirsk, Russia 34Institute for High Energy Physics (IHEP), Protvino, Russia

v 35Universitat de Barcelona, Barcelona, Spain 36Universidad de Santiago de Compostela, Santiago de Compostela, Spain 37European Organization for Nuclear Research (CERN), Geneva, Switzerland 38Ecole Polytechnique F´ed´erale de Lausanne (EPFL), Lausanne, Switzerland 39Physik-Institut, Universit¨atZ¨urich,Z¨urich,Switzerland 40Nikhef National Institute for Subatomic Physics, Amsterdam, The Netherlands 41Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, The Netherlands 42NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine 43Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine 44University of Birmingham, Birmingham, United Kingdom 45H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom 46Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom 47Department of Physics, University of Warwick, Coventry, United Kingdom 48STFC Rutherford Appleton Laboratory, Didcot, United Kingdom 49School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom 50School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom 51Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom 52Imperial College London, London, United Kingdom 53School of Physics and Astronomy, University of Manchester, Manchester, United Kingdom 54Department of Physics, University of Oxford, Oxford, United Kingdom 55Massachusetts Institute of Technology, Cambridge, MA, United States 56University of Cincinnati, Cincinnati, OH, United States 57Syracuse University, Syracuse, NY, United States 58Pontif´ıciaUniversidade Cat´olica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to 2 59Institut f¨urPhysik, Universit¨atRostock, Rostock, Germany, associated to 11 aP.N. Lebedev Physical Institute, Russian Academy of Science (LPI RAS), Moscow, Russia bUniversit`adi Bari, Bari, Italy cUniversit`adi Bologna, Bologna, Italy dUniversit`adi Cagliari, Cagliari, Italy eUniversit`adi Ferrara, Ferrara, Italy f Universit`adi Firenze, Firenze, Italy gUniversit`adi Urbino, Urbino, Italy hUniversit`adi Modena e Reggio Emilia, Modena, Italy iUniversit`adi Genova, Genova, Italy jUniversit`adi Milano Bicocca, Milano, Italy kUniversit`adi Roma Tor Vergata, Roma, Italy lUniversit`adi Roma La Sapienza, Roma, Italy mUniversit`adella Basilicata, Potenza, Italy nLIFAELS, La Salle, Universitat Ramon Llull, Barcelona, Spain oIFIC, Universitat de Valencia-CSIC, Valencia, Spain pHanoi University of Science, Hanoi, Viet Nam qUniversit`adi Padova, Padova, Italy rUniversit`adi Pisa, Pisa, Italy sScuola Normale Superiore, Pisa, Italy

vi 1 Introduction

Mesons are colourless objects composed of a -antiquark pair bound via the . Measurements of meson provide observables that can be compared to theoretical predictions. For the case of B mesons, precision measurements have been reported in recent years by several experiments [1–3]. In contrast, few precision D meson mass measurements exist. For the D0 meson1 the current average of M(D0) = 1864.91 ± 0.17 MeV/c2, quoted by the Review of Physics [4], is dominated by the measurements of the CLEO [5] + + and KEDR [6] collaborations. Current knowledge of the masses of the D and Ds mesons, and the mass splitting between these states, is more limited. The most precise determination of the D+ mass is made by the KEDR collaboration [6] resulting in M(D+) = 1869.53±0.49 (stat) ±0.20 (syst) MeV/c2. In addition, two measurements of the mass splitting between the D+ and D0 mesons by the MRK2 [7] and LGW [8] collaborations have been reported. These are averaged [4] to give M(D+) − M(D0) = 4.76 ± 0.28 MeV/c2. + 2 No absolute measurement of the Ds mass with a precision better than the MeV/c level exists and the reported values are not in good agreement [4]. More precise measurements of the mass difference relative to the D+ meson have been reported by several collaborations + + 2 [9–13]. These are averaged [4] to give M(Ds ) − M(D ) = 98.85 ± 0.25 MeV/c . The + 2 fit of open mass data [4] leads to M(Ds ) = 1968.49 ± 0.32 MeV/c . Though this value is significantly more precise than the direct measurement, it would still dominate the + + + systematic uncertainty on the measurement of the Bc mass in the Bc → J/ψDs decay mode [14]. Recent interest in the D0 mass has been driven by the observation of the X(3872) state, first measured by the [15] and subsequently confirmed elsewhere [16–20] . This state, with J PC = 1++ [21], does not fit well into the picture, and exotic interpretations have been suggested: for example that it is a [22] or a loosely bound deuteron-like D∗0D0 ‘’ [23]. For the latter interpretation to be valid, the mass of the X(3872) state should be less than the sum of the D∗0 and D0 masses. Using the fitted value of the D0 mass and the measured values for the other quantities quoted in Ref. [4], the (EB) in this interpretation can be estimated to be

0 ∗0 EB = M(D D ) − M(X(3872)) = 2M(D0) + ∆M(D∗0 − D0) − M(X(3872)) = 0.16 ± 0.32 MeV/c2.

Therefore, the issue of whether the X(3872) can be a bound molecular state remains open. To clarify the situation, more precise measurements of both the X(3872) and D0 masses are needed. In this paper, a measurement of the D0 mass using the D0 → K+K−K−π+ decay mode is reported. This mode has a relatively low energy release, Q-value, defined as the difference between the mass of the D meson and the sum of the masses of the daughter

1The inclusion of charge conjugate states is implied.

1 . Consequently, systematic uncertainties due to the calibration of the momentum scale of the detector are reduced. Other four-body D0 decay modes are used to provide a + 0 + + cross-check of the result. In addition, precision measurements of the D −D and Ds −D mass differences are made. For the mass difference measurements the D0 → K+K−π+π− + + − + mode is used, together with the D(s) → K K π decay, since these modes have similar Q-values.

2 Detector and dataset

−1 The analysis uses data, corresponding to an√ integrated luminosity of 1.0 fb , collected in pp collisions at a centre-of-mass energy of s = 7 TeV by the LHCb experiment during 2011. The detector response is studied using a simulation. -proton collisions are generated using Pythia 6.4 [24] with the configuration described in Ref [25]. Particle decays are then simulated by EvtGen [26] in which final state is generated using Photos [27]. The interaction of the generated particles with the detector and its response are implemented using the Geant4 toolkit [28] with the settings described in Ref. [29]. The LHCb detector [30] is a single-arm forward spectrometer covering the pseudo- rapidity range 2 < η < 5. It includes a high precision tracking system consisting of a silicon-strip vertex detector surrounding the pp interaction region, a large-area silicon-strip detector located upstream of a dipole magnet with a bending power of about 4 Tm, and three stations of silicon-strip detectors and straw drift tubes placed downstream. The polarity of the dipole magnet is reversed at intervals that correspond to roughly 0.1 fb−1 of collected data in order to minimize systematic uncertainties. The combined tracking system has momentum resolution ∆p/p that varies from 0.4% at 5 GeV/c to 0.6% at 100 GeV/c, and impact parameter resolution of 20 µm for tracks with high transverse momentum (pT). Charged are identified using two ring-imaging Cherenkov detectors. , and hadron candidates are identified by a calorimeter system consisting of scintillating-pad and pre-shower detectors, an electromagnetic calorimeter and a hadronic calorimeter. are identified by a system composed of alternating layers of iron and multiwire proportional chambers. The trigger [31] consists of a hardware stage, based on information from the calorimeter and systems, followed by a software stage that applies a full event reconstruction. Samples of open charm mesons produced directly in the primary pp interaction (refered to as ‘prompt’) and in semileptonic decays of b-hadrons are selected by the trigger. Though the prompt sample is larger in size, cuts on the decay time of the D meson are applied at the trigger level to reduce the output rate. As the reconstructed mass and decay time are correlated, these cuts bias the mass measurement. In contrast, no cuts on the D decay time are applied at the trigger level for the semileptonic sample, which is therefore used for this analysis. The measurements require the momenta of the final state particles to be determined accurately. The procedure used to calibrate the momentum scale of the tracking system for this study is discussed in detail in Ref. [32]. It is based upon large calibration samples

2 of B+ → J/ψK+ and J/ψ → µ+µ− decays collected concurrently with the dataset used for this analysis. The use of the large J/ψ dataset allows to correct for variations of the momentum scale at the level of 10−4 or less that occur over the course of the data-taking period whilst the use of the B+ → J/ψK+ allows the momentum scale to be determined as a function of the K+ kinematics. The accuracy of the procedure has been checked 0 using other fully reconstructed B decays together with two-body Υ(nS) and KS decays. In each case the deviation of the measured mass from the expected value is converted to an estimate of the bias on the momentum scale (α) taking into account relativistic kinematics and QED radiative corrections. The largest value of |α| found in these studies 0 + − is 0.03 % for the KS → π π decay mode. Conservatively, this is taken as the uncertainty on the calibrated momentum scale. This leads to the largest contribution to the systematic uncertainty on the mass measurements.

3 Selection

The selection uses only well reconstructed charged particles that traverse the entire tracking system. All charged particles are required to be within the angular acceptance of the spectrometer. This corresponds to 300 mrad in the bending plane of the dipole magnet and 250 mrad in the orthogonal plane. In addition, the final state particles are required to have pT greater than 300 MeV/c. Further background suppression is achieved by exploiting the fact that the products of heavy flavour decays have a large distance of closest approach (‘impact parameter’) with respect to the pp interaction vertex in which they were produced. The impact parameter χ2 with respect to any primary vertex is required to be larger than nine. Fake tracks created by the reconstruction are suppressed by cutting on the output of a neural network trained to discriminate between these and real particles. This cut also removes candidates where one of the charged hadrons has decayed in flight. To select well-identified () the difference in the logarithms of the global likelihood of the () hypothesis relative to the pion (kaon) hypothesis provided by the ring-imaging Cherenkov detectors is required to be greater than five (zero). Charged particles selected in this way are combined to form D0 → K+K−π+π−, 0 + − − + + + − + D → K K K π and D(s) → K K π candidates. To eliminate kinematic reflections due to misidentified pions, the of at least one kaon pair is required to be within ±12 MeV/c2 of the nominal value of the φ meson mass [4]. This requirement means that the D meson sample is dominated by decays containing an intermediate φ meson. A fit requiring the final state particles to originate from a common point is made and the χ2 per degree of freedom (χ2/ndf) of this fit is required to be less than five. In order to remove poorly reconstructed candidates, a cut is made on the uncertainty of the reconstructed invariant mass estimated by propagation of the individual track covariance matrices. The value of this cut depends on the decay mode under consideration and is chosen such that the bulk of the distribution is kept and only events in the tail are rejected. In a few percent of the events the reconstruction procedure gives rise to duplicate candidates. Therefore, if two or more candidates that are separated by less than 0.05 in

3 pseudorapidity and 50 mrad in azimuthal angle are found within one event, only that with the best D vertex χ2 is kept. Each candidate D meson, selected in this way, is combined with a well-identified muon that is displaced from the pp interaction vertex (impact parameter χ2 > 4) and that has pT larger than 800 MeV/c to form a B candidate. A fit is made requiring the muon and the D candidate to originate from a common point and the χ2 per degree of freedom of this fit is required to be less than five. To select semileptonic B decays, the invariant mass of the B candidate is required to be in the range 2.5 − 6.0 GeV/c2. In principle, the large combinatorial background can be further reduced by cutting on the decay time of the D meson, but due to the correlation between the decay time and the mass, this cut would bias the mass distribution. Therefore, a cut requiring significant displacement between the b-hadron decay vertex and the associated pp interaction vertex is applied. This achieves high signal purity whilst not biasing the distribution of the D decay time.

4 Fit Results

The D meson masses are determined by performing extended unbinned maximum likelihood fits to the invariant mass distributions. In these fits the background is modelled by an exponential function and the signal by the sum of a Crystal Ball [33] and a Gaussian function. The Crystal Ball component accounts for the presence of the QED radiative tail. Alternative models for both the signal and background components are considered as part of the studies of the systematic uncertainties. The model for the signal shape contains six parameters: • a common mean value for the Gaussian and Crystal Ball components;

• the widths of the Gaussian (σG) and the Crystal Ball (σCB) components; • the transition point (a) and exponent (n) of the Crystal Ball component;

• the relative fraction of the Crystal Ball (fCB) component.

To reduce the number of free parameters in the fit, a, n and fCB together with the ratio of σCB to σG, are fixed using a simulation that has been tuned to reproduce the mass resolution observed in data for the B+ → J/ψK+ and B+ → J/ψK+π−π+ decay modes. By fixing the ratio of σCB to σG the resolution model is constrained up to an overall resolution scale factor that is close to unity. The Crystal Ball function describes the effect of the radiative tail far from the peak well. However, close to the peak its shape is still Gaussian, which results in a bias on the fitted mass that scales with the Q-value of the decay mode. This effect is studied using Photos [27] to model the effect of QED radiative corrections. The size of the bias is found to be 0.03 ± 0.01 MeV/c2 for the D0 → K+K−K−π+ mode. For the D0 → K+K−π+π−, + + − + + + − + 2 D → K K π and Ds → K K π decay modes a value of 0.06 ± 0.01 MeV/c is found. These values are used to correct the mass measurements. The effect cancels in the measurement of the mass differences.

4 ) 800 ) 2 2

c c 250 700 LHCb (a) LHCb (b)

600 200

500 150 400

300 100

200 Candidates/ (2 MeV/ Candidates/ (2 MeV/ 50 100

0 0 1820 1840 1860 1880 1900 1920 1820 1840 1860 1880 1900 1920 − − − M(K+K π+ π −) [MeV/c2] M(K+ K K π+) [MeV/c2] 6 6 4 4 2 2 pull 0 pull 0 -2 -2 -4 -4 -6 -6

Figure 1: Invariant mass distributions for the (a) K+K−π+π− and (b) K+K−K−π+ final states. In each case the result of the fit described in the text is superimposed (solid line) together with the background component (dotted line). The pull, i.e. the difference between the fitted and measured value divided by the uncertainty on the measured value, is shown below each plot.

Table 1: Signal yields, mass values, resolution scale factors and binned χ2/ndf (using 100 bins) obtained from the fits shown in Fig. 1 and Fig. 2 together with the values corrected for the effect of QED radiative corrections as described in the text.

Fitted mass Corrected mass Resolution Decay mode Yield χ2/ndf [MeV/c2] [MeV/c2] scale factor D0 → K+K−π+π− 4608 ± 89 1864.68 ± 0.12 1864.74 ± 0.12 1.031 ± 0.021 0.83 D0 → K+K−K−π+ 849 ± 36 1864.73 ± 0.15 1864.75 ± 0.15 0.981 ± 0.042 0.92 D+ → K+K−π+ 68, 787 ± 321 1869.44 ± 0.03 1869.50 ± 0.03 0.972 ± 0.003 + + − + 2.5 Ds → K K π 248, 694 ± 540 1968.13 ± 0.03 1968.19 ± 0.03 0.971 ± 0.002

The resulting fits for the D0 decay modes are shown in Fig. 1 and that for the K+K−π+ final state in Fig. 2. The values obtained in these fits are summarized in Table 1. The + + resulting values of the D and Ds masses are in agreement with the current world averages. These modes have relatively large Q-values and consequently the systematic uncertainty due to the knowledge of the momentum scale is at the level of 0.3 MeV/c2. Hence, it is chosen not to quote these values as measurements. Similarly, the systematic uncertainty due to the momentum scale for the D0 → K+K−π+π− mode is estimated to be 0.2 MeV/c2 and the measured mass in this mode is not used in the D0 mass determination. The quality of the fits is judged from the χ2/ndf, quoted in Table 1, and the fit residuals. It has been checked using simulated pseudo-experiments that the sizeable trends seen in the residuals for the K+K−π+ mode, where the dataset is largest, do not bias the mass difference measurement. The fitted resolution scale factors are all within a few

5 ) 2 c 30000 LHCb

25000

20000

15000

10000 Candidates/ (2 MeV/ 5000

0 1850 1900 1950 2000 − M(K+K π+) [MeV/c2] 6 4 2 pull 0 -2 -4 -6 Figure 2: Invariant mass distribution for the K+K−π+ final state. The result of the fit described in the text is superimposed (solid line) together with the background component (dotted line). The pull, i.e. the difference between the fitted value and the measured value divided by the uncertainty, is shown below the plot.

percent of unity, indicating that the calibration parameters obtained from the B+ study are applicable in this analysis. The uncertainties on the masses reported by the fits are in good agreement with the results obtained in pseudo-experiments. Using the values in Table 1, the mass differences are evaluated to be M(D+) − M(D0) = 4.76 ± 0.12 (stat) MeV/c2, + + 2 M(Ds ) − M(D ) = 98.68 ± 0.03 (stat) MeV/c , where the uncertainties are statistical only.

5 Systematic uncertainties

To evaluate the systematic uncertainty, the complete analysis is repeated, including the track fit and the momentum scale calibration when needed, varying within their uncertainties the parameters to which the mass determination is sensitive. The observed changes in the central values of the fitted masses relative to the nominal results are assigned as systematic uncertainties. The dominant source of uncertainty is the limited knowledge of the momentum scale. The mass fits are repeated with the momentum scale varied by ±0.03 %. A further

6 Table 2: Systematic uncertainties (in MeV/c2) on the mass measurements and on their differences.

0 + 0 + + Source of uncertainty M(D ) M(D ) − M(D ) M(Ds ) − M(D ) Momentum scale 0.09 0.04 0.04 Energy loss correction 0.03 0.06 <0.01 K± mass 0.05 <0.01 <0.01 Signal model 0.02 <0.01 <0.01 Background model <0.01 <0.01 <0.01 Quadratic sum 0.11 0.07 0.04

uncertainty is related to the understanding of the energy loss in the material of the tracking system. The amount of material traversed in the tracking system by a particle is known to 10 % accuracy [34]. Therefore, the magnitude of the energy loss correction in the reconstruction is varied by ±10 %. Other uncertainties arise from the fit model. To evaluate the impact of the signal model, a fit is performed where all signal parameters are fixed according to the values found in the simulation and a second fit where the parameters σG and σCB are allowed to vary while keeping the relative fraction, fCB, of the two components fixed. The larger of the differences to the default fit result is assigned as an estimate of the systematic uncertainty. Similarly the effect of the background modelling is estimated by replacing the exponential function with a first-order Chebychev polynomial. The shifts of the mass values observed in these tests are generally much smaller than 0.01 MeV/c2 and are assigned as systematic uncertainties. For the K+K−π+ fit further cancellation occurs in the mass difference. It is concluded that the details of the fit model have little effect on the presented measurements. An additional uncertainty arises from the knowledge of the value of the K+ mass, 2 mK± = 493.677 ± 0.016 MeV/c [4]. The effect of this uncertainty on the measurements has been evaluated from simulation studies. The systematic uncertainties on the measured masses and mass differences are sum- marized in Table 2. The uncertainties related to the momentum scale and energy loss correction are fully correlated between the measurements. Various cross-checks of the measurements are made. Two checks are related to the knowledge of the tracking system alignment. First, a study has been performed where particle trajectories are reconstructed without using the information related to the tracking detector located before the entrance of the spectrometer magnet. This information is not required to form a track but improves the momentum resolution by 10 − 20 %. The second test is to vary the track slopes in the vertex detector by the uncertainty of 2 × 10−4 on the length scale of the detector described in Ref. [35]. The results obtained in these studies are consistent with those presented here and no additional uncertainty is assigned. A further check for the D0 mass measurement is the comparison of the measured mass in the D0 → K+K−K−π+ mode with that obtained in the three other four-body modes. Systematic effects related to the momentum scale will affect modes with a high Q-value

7 more than those with low Q-values. The relationship between the reconstructed mass (m) and the momentum scale (α) after a first-order Taylor expansion in m2/p2 is

m2 − f m2 = true + f, (1) (1 − α)2 where X m2 f = p i , (2) pi p is the total momentum of the decaying meson and pi and mi are the momenta and masses of the daughter particles. This formalism assumes that there are no additional differences affecting the momentum scale between the modes such as differences in track kinematics or the effect of QED radiative corrections. For each decay mode the average value of f is obtained from the data using the sPlot technique [36] with the mass as the control variable to subtract the effect of background. The values obtained in this way are in good agreement with those found in the simulation. In Fig. 3 the measured D0 mass is plotted versus f for the four-body decay modes studied here. The shaded area on this plot corresponds to the assigned systematic uncertainty of 0.03 % on the momentum scale. Though there is evidence of a systematic effect for the low f-value modes it is accounted for by the assigned uncertainty.

] 1866 2 c

1865.5 LHCb ) [MeV/ 0

M(D 1865

− − 1864.5 0 + + − → π 0 + + − D K K K − D → K K π π D0 → K π+ π+ π − D0 → π+π − π+π − 1864

1863.5 1 2 3 f [GeV2/c4]

Figure 3: Measured D0 mass versus f as defined in Eq. 2. The (yellow) shaded area corresponds to a systematic uncertainty on the momentum scale of 0.03 % centred on the result for the D0 → K+K−K−π+ mode (horizontal dashed line). Only the D0 → K+K−K−π+ mode, where the systematic uncertainty is lowest, is used to determine the D0 mass.

8 Table 3: LHCb measurements, compared to the best previous measurements and to the results of a global fit to available open charm mass data. The quoted uncertainties are the quadratic sums of the statistical and systematic contributions. All values are in MeV/c2.

LHCb Best previous Quantity PDG fit [4] measurement measurement M(D0) 1864.75 ± 0.19 1864.85 ± 0.18 [5] 1864.86 ± 0.13 M(D+) − M(D0) 4.76 ± 0.14 4.7 ± 0.3 [7] 4.76 ± 0.10 + + M(Ds ) − M(D ) 98.68 ± 0.05 98.4 ± 0.3 [10] 98.88 ± 0.25

The dataset has also been divided according to the magnet polarity and data-taking period and for the charged modes by the sign of the product of the magnet polarity and the D meson charge. In addition, for modes where the event samples are sizable the measurements are repeated in bins of the D meson kinematic variables. None of these tests reveal any evidence of a systematic bias.

6 Summary

Measurements of D meson masses and mass differences have been performed using pp −1 collision data, corresponding√ to an integrated luminosity of 1.0 fb collected at a centre- of-mass energy of s = 7 TeV with the LHCb detector. The results are

M(D0) = 1864.75 ± 0.15 (stat) ± 0.11 (syst) MeV/c2, M(D+) − M(D0) = 4.76 ± 0.12 (stat) ± 0.07 (syst) MeV/c2, + + 2 M(Ds ) − M(D ) = 98.68 ± 0.03 (stat) ± 0.04 (syst) MeV/c . The dominant systematic uncertainty is related to the knowledge of the momentum scale. As shown in Table 3, these measurements are in agreement with previous measurements. The results for the mass differences have smaller uncertainty than any previously reported value. The measured value of the D0 mass has a similar precision to the published CLEO result [5]. Including this result in the determination of the X(3872) binding energy given 2 in Section 1 gives EB = 0.09 ± 0.28 MeV/c . This reinforces the conclusion that if the X(3872) state is a molecule it is extremely loosely bound. The measurements presented here, together with those given in Ref. [4] for the D+ and 0 + 0 + + D mass, and the mass differences M(D ) − M(D ), M(Ds ) − M(D ) can be used to + determine a more precise value of the Ds mass

+ 2 M(Ds ) = 1968.19 ± 0.20 ± 0.14 ± 0.08 MeV/c , where the first uncertainty is the quadratic sum of the statistical and uncorrelated system- atic uncertainty, the second is due to the momentum scale and the third due to the energy

9 loss. This value is consistent with, but more precise than, that obtained from the fit to + 2 open charm mass data, M(Ds ) = 1968.49 ± 0.32 MeV/c [4].

Acknowledgements

We express our gratitude to our colleagues in the CERN accelerator departments for the excellent performance of the LHC. We thank the technical and administrative staff at the LHCb institutes. We acknowledge support from CERN and from the national agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); NSFC (China); CNRS/IN2P3 and Region Auvergne (France); BMBF, DFG, HGF and MPG (Germany); SFI (Ireland); INFN (Italy); FOM and NWO (The Netherlands); SCSR (Poland); ANCS/IFA (Romania); MinES, Rosatom, RFBR and NRC “Kurchatov Institute” (Russia); MinECo, XuntaGal and GENCAT (Spain); SNSF and SER (Switzerland); NAS Ukraine (Ukraine); STFC (United Kingdom); NSF (USA). We also acknowledge the support received from the ERC under FP7. The Tier1 computing centres are supported by IN2P3 (France), KIT and BMBF (Germany), INFN (Italy), NWO and SURF (The Netherlands), PIC (Spain), GridPP (United Kingdom). We are thankful for the computing resources put at our disposal by Yandex LLC (Russia), as well as to the communities behind the multiple open source software packages that we depend on.

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